Long-Wavelength Oscillations and the Gallex Solar Neutrino Signal
arXiv:hep-ph/9207257 · doi:10.1103/PhysRevLett.69.3135
Abstract
The recently reported solar neutrino signal in the Ga GALLEX detector adds a new dimension to the solar neutrino puzzle, complementing the previously known signals in Cl and water-Cherenkov detectors. Possible explanations for this new signal in terms of matter-enhanced neutrino oscillations (MSW effect) are already awaiting in the literature. We point out here that long-wavelength vacuum oscillations can furnish an alternative explanation of all three signals simultaneously; such solutions give neutrino spectra with distinctive energy dependence and seasonal time dependence. %This is a Revtex file, which is Latex-based but depends upon inputting the %Revtex style files distributed by APS/Physical Review. For more information, %contact Peggy Sutherland at [email protected], phone (516) 349-7800 ext 674
11 pages, 3 figures available by conventional mail or fax, MAD/PH/708
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